Abstract
In this paper it is shown that in the process of formation of a single star system favorable conditions are created for the appearance of the planetary system due to the collision of the oppositely moving condensed dust zones from the newly born star and falling onto it from the periphery. A hypothetical version of the possible structure of the core of a single star born in a rarefied gas-dust cloud, explaining the cause of the mismatch of the axis of rotation of the star and the dipole magnetic field, is proposed. An assumption is made about the causes of the appearance of a directed orbital motion of planets that are not related to external perturbations of the initial gas-dust cloud.
Highlights
At the present stage of evolution of the universe, gas-dust clouds in outer space form as a result of emissions or explosions of stars later generations
The generalized approach made it possible to take a case in which galaxies were "dust particles" and show the premature introduction of the new category of "dark energy" into physics
The goal set in this paper is to identify the main characteristic features of the process of gravitational compression in the space of a rarefied gas-dust cloud on the basis of a schematic description of the resulting physical processes
Summary
At the present stage of evolution of the universe, gas-dust clouds in outer space form as a result of emissions or explosions of stars later generations. The inversion of the density, when the density becomes maximal in the central zone, occurs only with the appearance of short-range repulsive forces continuously distributed throughout the volume of the cloud Such an undeniable position, unusual for theoreticians, about the distribution of density of a dust cloud which self-contracts due to gravitational forces in the process of its compression (rather than at the end of the process) is an interesting fact in itself, and serves as a key link in the initial stage of separation of heavy elements, even before the stage of formation of the planetary belt of a single star, at which separation develops and terminates. This work is devoted to the consideration of such new schemes of gravitational interactions during the spontaneous compression of a gas-dust cloud, including the study of the features of the formation of a star and a planetary belt in the vicinity of a burning star and the causes of the appearance of the considered physical processes are analyzed. The twisting is caused not by external perturbations, but by the kinetics of the internal processes of a compressed rarefied gas-dust cloud
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